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- W1891036154 abstract "Based on the concept of orbital stability introduced by G. W. Hill, a method is presented to facilitate the determination of the orbital stability of solutions to the planar elliptic restricted problem of three bodies. The invariant relation introduced by Szebehely and Giacaglia (1964) contains an integral which is expanded here about a Keplerian solution to the problem. If the expansion converges, it can be used to determine the conditions for Hill stability. With it one can also define stability in a periodic sense." @default.
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- W1891036154 date "1978-01-01" @default.
- W1891036154 modified "2023-09-27" @default.
- W1891036154 title "Orbital Stability in the Elliptic Restricted Three Body Problem" @default.
- W1891036154 cites W1970508028 @default.
- W1891036154 doi "https://doi.org/10.1007/978-94-009-9809-4_39" @default.
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